Grid of 1D models for Mg line formation

DOI

Mg is the alpha element of choice for Galactic population and chemical evolution studies as it is easily detectable in all late-type stars. Such studies require precise elemental abundances, and thus departures from LTE need to be accounted for.

Identifier
DOI http://doi.org/10.26093/cds/vizier.35860120
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/586/A120
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/586/A120
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/586/A120
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/586/A120
Provenance
Creator Osorio Y.; Barklem P.S.
Publisher CDS
Publication Year 2016
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Interdisciplinary Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy